【作者单位】1Institute of Theoretical Physics, Shanxi University, Taiyuan 030006, People's Republic of China;jsniu@sxu.edu.cn, hfxue@tynu.edu.cn;2State Key Laboratory of Quantum Optics and Quantum Optics Devices, Shanxi University, Taiyuan 030006, People's Republic of China;3Department of Physics, Taiyuan Normal University, Jinzhong 030619, People's Republic of China;4Institute of Computational and Applied Physics, Taiyuan Normal University, Jinzhong 030619, People's Republic of China
【年份】2023
【卷号】Vol.166 No.2
【页码】43
【摘要】 Harmonics are quite common in pulsating stars. They are always considered to mimic the behaviors of their independent parent pulsation modes, and are not taken for key information in asteroseismology. Here, we report an SX Phoenicis star XX Cygni, wh...
